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Python libraries specifically designed for astronomical data analysis, coordinate calculations, and unit handling.
Distinct from Python Libraries: Distinct from Python Libraries: focuses on astronomy-specific functionality, not general-purpose Python tools.
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This project is a suite of software for radio interferometry imaging, specialized in the processing, analysis, and reconstruction of Very Long Baseline Interferometry (VLBI) observations. It provides tools for reconstructing images from interferometry data using regularized maximum likelihood methods and managing the end-to-end data processing pipeline from raw visibilities to final images. The software distinguishes itself with a dedicated interstellar scattering simulator that models thin-screen scattering effects and applies scattering kernels to radio images. It also features a radio imag
Provides a library for computing polarimetric flux, circular statistics, and bootstrap confidence intervals for astronomical data.
Astropy is a core Python library for astronomy, providing a unified framework for astronomical data analysis, coordinate and time computations, and physical constants and unit handling. It is designed as a standard tool for the astronomy community, enabling consistent reading, processing, and visualization of FITS files and ASCII tables through a modular subpackage system that shares common interfaces and conventions. The library distinguishes itself through broad interoperability across astronomy software, establishing shared protocols for data exchange and collaboration. It includes a coord
Serves as a standard Python library for astronomical data analysis, coordinate calculations, and unit handling.